Fig. 1 from A Young Cluster of Galaxies at z = 2.5

Image Details

View Article Bookmark & Share

Choose export citation format:

Export Citation

Hi-Resolution

Export to PDF PPT Format

A Young Cluster of Galaxies at z = 2.5

Authors: M. A. Malkan, H. Teplitz, and I. S. McLean

Malkan, Teplitz, & McLean 1996 The Astrophysical Journal Letters 468 L9.

Provider: AAS Journals

Caption: Fig. 1.

Observed LRIS/Keck spectrum of MTM 095355+545428, boxcar smoothed by 3 pixels (7.5 Å). Arrows indicate the wavelengths of the strongest expected UV stellar and interstellar absorption lines for a starburst galaxy. The two negative‐going features are due to poor subtraction of sky lines.

Other Images in This Article

Copyright and Terms & Conditions